output
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2012 · astro-ph.COShow all

34 papers · 2 filters

astro-ph.CO2012★ 134 cited

The Carnegie-Irvine Galaxy Survey. III. The Three-Component Structure of Nearby Elliptical Galaxies

Song Huang, Luis C. Ho, Chien Y. Peng +2

Motivated by recent developments in our understanding of the formation and evolution of massive galaxies, we explore the detailed photometric structure of a representative sample o…

astro-ph.CO2012★ 41 cited

Subhaloes gone Notts: Spin across subhaloes and finders

Julian Onions, Yago Ascasibar, Peter Behroozi +15

We present a study of a comparison of spin distributions of subhaloes found associated with a host halo. The subhaloes are found within two cosmological simulation families of Milk…

astro-ph.CO2012★ 27 cited

Exploring the Cosmic Reionization Epoch in Frequency Space: An Improved Approach to Remove the Foreground in 21 cm Tomography

Jingying Wang, Haiguang Xu, Tao An +7

Aiming to correctly restore the redshifted 21 cm signals emitted by the neutral hydrogen during the cosmic reionization processes, we re-examine the separation approaches based on…

astro-ph.CO2012★ 26 cited

Kinematics of the Compact Symmetric Object OQ 208 revisited

Fang Wu, Tao An, Willem A. Baan +6

Aims. A long timeline kinematic study of the archetypal CSO OQ 208 sheds light on the physical properties of the most compact radio sources. Methods. Archival data from the VLBA at…

astro-ph.CO2012★ 24 cited

Stellar mass versus stellar velocity dispersion: which is better for linking galaxies to their dark matter halos?

Cheng Li, Lixin Wang, Y. P. Jing

It was recently suggested that, compared to its stellar mass (M*), the central stellar velocity dispersion (sigma*) of a galaxy might be a better indicator for its host dark matter…

astro-ph.CO2012★ 215 cited

The Dynamic Evolution of Young Extragalactic Radio Sources

Tao An, Willem A. Baan

The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth stages of the radio luminosity versus size of the source. The interaction of the…

astro-ph.CO2012★ 45 cited

The Baldwin effect in the narrow emission lines of AGNs

Kai Zhang, Ting-Gui Wang, C. Martin Gaskell +1

The anti-correlations between the equivalent widths of emission lines and the continuum luminosity in AGNs, known as the Baldwin effect are well established for broad lines, but ar…

astro-ph.CO2012★ 46 cited

Galaxies going MAD: The Galaxy-Finder Comparison Project

Alexander Knebe, Noam I. Libeskind, Frazer Pearce +8

With the ever increasing size and complexity of fully self-consistent simulations of galaxy formation within the framework of the cosmic web, the demands upon object finders for th…

astro-ph.CO2012★ 28 cited

Constraining the substructure of dark matter haloes with galaxy-galaxy lensing

Ran Li, Houjun Mo, Zuhui Fan +2

With galaxy groups constructed from the Sloan Digital Sky Survey (SDSS), we analyze the expected galaxy-galaxy lensing signals around satellite galaxies residing in different host…

astro-ph.CO2012★ 20 cited

The distribution of faint satellites around central galaxies in the CFHT Legacy Survey

Chunyan Jiang, Yipeng Jing, Cheng Li

We investigate the radial number density profile and the abundance distribution of faint satellites around central galaxies in the low redshift universe using the CFHT Legacy Surve…

astro-ph.CO2012★ 53 cited

What governs the bulk velocity of the jet components in active galactic nuclei?

Bo Chai, Xinwu Cao, Minfeng Gu

We use a sample of radio-loud active galactic nuclei (AGNs) with measured black hole masses to explore the jet formation mechanisms in these sources. Based on the Königl's inhomoge…

astro-ph.CO2012★ 165 cited

A Re-examination of Galactic Conformity and a Comparison with Semi-analytic Models of Galaxy Formation

Guinevere Kauffmann, Cheng Li, Wei Zhang +1

The observed correlation between star-formation in central galaxies and in their neighbours (a phenomenon dubbed galactic conformity) is in need of a convincing physical explanatio…

astro-ph.CO2012★ 5 cited

Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario

Zhigang Li, Pengjie Zhang, Xuelei Chen

We search for the dark flow induced diffuse kinetic Sunyaev Zel'dovich (kSZ) effect through CMB-galaxy cross correlation. Such angular correlation is anisotropic, with a unique $co…

astro-ph.CO2012★ 69 cited

ALFALFA HI Data Stacking III. Comparison of environmental trends in HI gas mass fraction and specific star formation rate

Silvia Fabello, Guinevere Kauffmann, Barbara Catinella +3

It is well known that both the star formation rate and the cold gas content of a galaxy depend on the local density out to distances of a few Megaparsecs. In this paper, we compare…

astro-ph.CO2012★ 86 cited

Satellites and Haloes of Dwarf Galaxies

Laura V. Sales, Wenting Wang, Simon D. M. White +1

We study the abundance of satellite galaxies as a function of primary stellar mass using the SDSS/DR7 spectroscopic catalogue. In contrast with previous studies, which focussed mai…

astro-ph.CO2012★ 22 cited

The Evolution and Star Formation History of M33

Xiaoyu Kang, Ruixiang Chang, Jun Yin +4

We construct a parameterized model to explore the main properties of the star formation history of M33. We assume that the disk originates and grows by the primordial gas infall an…

astro-ph.CO2012★ 179 cited

Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data

Marcello Cacciato, Frank C. van den Bosch, Surhud More +2

We simultaneously constrain cosmology and galaxy bias using measurements of galaxy abundances, galaxy clustering and galaxy-galaxy lensing taken from the Sloan Digital Sky Survey.…

astro-ph.CO2012★ 84 cited

Constraining Extended Gamma-ray Emission from Galaxy Clusters

Jiaxin Han, Carlos S. Frenk, Vincent R. Eke +5

Cold dark matter models predict the existence of a large number of substructures within dark matter halos. If the cold dark matter consists of weakly interacting massive particles,…

astro-ph.CO2012★ 24 cited

Bulk flow of halos in ΛCDM simulation

Ming Li, Jun Pan, Liang Gao +10

Analysis of the Pangu N-body simulation validates that the bulk flow of halos follows a Maxwellian distribution which variance is consistent with the prediction of the linear theor…

astro-ph.CO2012★ 47 cited

Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology

Pengjie Zhang, Jun Pan, Yi Zheng

Massive spectroscopic surveys will measure the redshift space distortion (RSD) induced by galaxy peculiar velocity to unprecedented accuracy. We develop a new method to improve the…

astro-ph.CO2012★ 73 cited

Cosmological Constraints from a Combination of Galaxy Clustering & Lensing -- II. Fisher Matrix Analysis

Surhud More, Frank van den Bosch, Marcello Cacciato +3

We quantify the accuracy with which the cosmological parameters characterizing the energy density of matter (Ω_m), the amplitude of the power spectrum of matter fluctuations (σ_8),…

astro-ph.CO2012★ 237 cited

Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework

Frank van den Bosch, Surhud More, Marcello Cacciato +2

We present a new method that simultaneously solves for cosmology and galaxy bias on non-linear scales. The method uses the halo model to analytically describe the (non-linear) matt…

astro-ph.CO2012★ 30 cited

Two in one? A possible dual radio-emitting nucleus in the quasar SDSS J1425+3231

S. Frey, Z. Paragi, T. An +1

The radio-emitting quasar SDSS J1425+3231 (z=0.478) was recently found to have double-peaked narrow [O III] optical emission lines. Based on the analysis of the optical spectrum, P…

astro-ph.CO2012★ 14 cited

The growth of the disk galaxy UGC8802

R. X. Chang, S. Y. Shen, J. L. Hou

The disk galaxy UGC8802 has high neutral gas content and a flat profile of star formation rate compared to other disk galaxies with similar stellar mass. It also shows a steep meta…